Calibration of CNEOS Fireball Velocities and the Robustness of Nominally Hyperbolic Events

arXiv:2609.06745 · astro-ph.EP, astro-ph.GA, astro-ph.IM · Submitted 2026-09-06 · Read on arXiv

astro-ph.EP, astro-ph.GA, astro-ph.IM

Submitted: 2026-09-06

Updated: 2026-09-06

Comments: 29 pages, 11 figures, 11 tables

License: http://creativecommons.org/licenses/by-sa/4.0/

The gist: The NASA/JPL CNEOS Fireball Data catalogue provides a near-global record of bright atmospheric entries but does not report per-event velocity covariance.

Terminology

Abstract

The NASA/JPL CNEOS Fireball Data catalogue provides a near-global record of bright atmospheric entries but does not report per-event velocity covariance. We calibrate its kinematic accuracy using 19 events with independent reference trajectories and use optical, satellite, radar, and infrasound catalogues as source-specific controls. For nine modern high-quality comparisons, the CNEOS-minus-reference speed residual has mean-1.00 km s-1 and standard deviation 0.86 km s-1; variance decomposition assigns 0.77 km s-1 to the CNEOS component. The radiant residuals have a 0.74 degree per-axis core plus one 16.3 degree outlier, so the extreme tail remains poorly determined. Seven of 354 complete CNEOS states are nominally hyperbolic without correction. A +0.9935 km s-1 atmospheric-stage shift produces five additional crossings, but these are treated only as sensitivity cases. Polar-IM (2026 April 1) is the strongest post-2018 CNEOS anomaly, whereas independent GLM-LI stereo solutions yield 57.3 +/- 2.0 and 56.7 +/- 3.0 km s-1, close to their direction-specific parabolic thresholds. We conclude that CNEOS can identify priority candidates, but secure interstellar classification requires an independent, uncertainty-bearing three-dimensional trajectory for the same event.

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